We also considered GR and EQG predictions for lensing effects due to SMBHs in other galaxies. We find that results of GR and EQG for the differential time delay between primary and secondary images could differ by an amount of more than one minute for distant SMBHs. The deviation between GR and EQG predictions for image angular positions mostly depends on the mass of black hole and it reminds us to what we found in [1]}. Very massive EQG black holes are like ordinary Schwarzschild black holes. However intermediate mass EQG black holes deviate significantly. This point should be discussed elsewhere.
